LAGER Lyα Luminosity Function at z ∼ 7: Implications for Reionization

被引:53
作者
Wold, Isak G. B. [1 ]
Malhotra, Sangeeta [1 ]
Rhoads, James [1 ]
Wang, Junxian [2 ,3 ]
Hu, Weida [2 ,3 ]
Perez, Lucia A. [4 ]
Zheng, Zhen-Ya [5 ]
Khostovan, Ali Ahmad [1 ]
Walker, Alistair R. [6 ]
Felipe Barrientos, L. [7 ,8 ]
Gonzalez-Lopez, Jorge [7 ,8 ,9 ]
Harish, Santosh [4 ]
Infante, Leopoldo [10 ]
Jiang, Chunyan [5 ]
Pharo, John [4 ]
Moya-Sierralta, Cristobal [7 ,8 ]
Bauer, Franz E. [7 ,8 ,11 ,12 ]
Galaz, Gaspar [7 ,8 ]
Valdes, Francisco [13 ]
Yang, Huan [10 ]
机构
[1] NASA, Goddard Space Flight Ctr, Astrophys Sci Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
[2] Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[3] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
[4] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
[5] Shanghai Astron Observ, CAS Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
[6] NSFs NOIRLab, Cerro Tololo Interamer Observ, Casilla 603, La Serena, Chile
[7] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Casilla 306, Santiago 22, Chile
[8] Pontificia Univ Catolica Chile, Fac Fis, Ctr Astroingn, Casilla 306, Santiago 22, Chile
[9] Univ Diego Portales, Nude Astron, Fac Ingn & Ciencias, Av Ejercito Libertador 441, Santiago, Chile
[10] Carnegie Inst Washington, Las Campanas Observ, Casilla 601, La Serena, Chile
[11] Millennium Inst Astrophys, Nuncio Monsefior Sotero Sanz 100,104, Santiago, Chile
[12] Space Sci Inst, 4750 Walnut St,Suite 205, Boulder, CO 80301 USA
[13] Natl Opt Astron Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA
基金
美国国家科学基金会; 日本学术振兴会; 日本科学技术振兴机构; 美国国家航空航天局; 英国科学技术设施理事会;
关键词
HUBBLE DEEP FIELD; EMITTING GALAXIES; COSMIC REIONIZATION; SPECTROSCOPIC CONFIRMATION; LYMAN BREAK; REDSHIFT; EVOLUTION; EMITTERS; EPOCH; CONSTRAINTS;
D O I
10.3847/1538-4357/ac4997
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new measurement of the Ly alpha luminosity function (LF) at redshift z = 6.9, finding moderate evolution from z = 5.7 that is consistent with a fully or largely ionized z similar to 7 intergalactic medium. Our result is based on four fields of the LAGER (Lyman Alpha Galaxies in the Epoch of Reionization) project. Our survey volume of 6.1 x 10(6) Mpc(3) is double that of the next largest z similar to 7 survey. We combine two new LAGER fields (WIDE12 and GAMA15A) with two previously reported LAGER fields (COSMOS and CDFS). In the new fields, we identify N = 95 new z = 6.9 Ly alpha emitter (LAEs) candidates, characterize our survey's completeness and reliability, and compute Ly alpha LFs. The best-fit Schechter LF parameters for all four LAGER fields are in good general agreement. Two fields (COSMOS and WIDE12) show evidence for a bright-end excess above the Schechter function fit. We find that the Ly alpha luminosity density declines at the same rate as the UV continuum LF from z = 5.7 to 6.9. This is consistent with an intergalactic medium that was fully ionized as early as redshift z similar to 7 or with a volume-averaged neutral hydrogen fraction of x (H I) < 0.33 at 1 sigma.
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页数:15
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